VPN技术在新疆地磁台阵中的应用

介绍了新疆地磁台阵的测点分布、测点设备构成情况以及运用VPN技术将地磁台阵观测系统接入地震行业网、VPN网络建设等情况。在新疆地磁台阵中应用VPN技术,实现了地震行业网对地磁台阵设备的远程管理和数据交换,随时获取数据信息,并能够对地震前后观测信息短临变化进行快速跟踪。     

可移动式磁通门台阵监测实用技术研究

现有的地磁台站(基准、基本台)网络、流动地磁监测网络监测模式各有其特点。地磁台站可以产出连续的地磁场三分量绝对观测数据,时间分辨率较高,但地磁台站间距较大,一般在200 km以上,显然空间分辨率相对较弱,对于中强地震孕震区内岩石圈     

地磁加卸载响应比方法最佳阈值研究

地磁加卸载响应比方法(LURR)是从测震学中移植过来的、用于地震中期分析预测的一种地磁学方法。笔者应用红山地震台地磁数字化观测数据进行了地磁加卸载响应比的计算分析,经过统计得出在阈值选择为3.0时对地震进行预测的效果比较好,其与地震的对应概率为42%。同时,笔者还认为可能受限于方法本身及外界因素,地磁加卸载响应比方法在进行地震预测时,其虚报率及漏报率较高。     

乌鲁木齐地磁台的观测与实践

乌鲁木齐地磁台的观测与实践高祥真，黄建明，王文德（中国新疆８３００１７乌鲁木齐地震台）豆前言乌鲁木齐台属国家１类地磁台，它始建于１９６５年，１９７０年正式投入观测。２０多年来，乌鲁木齐地磁台的观测工作已取得了一定的成绩，积累了大量的连续完整、准确可靠...     

地磁HHT频谱分析在地震预测中的应用

利用希尔伯特-黄变换方法,对成都、重庆、拉萨地磁台记录到的汶川MS 8.0地震、汶川地震余震地磁数据进行分析处理,发现在4级及以上中强度地震前3个月内地磁相对观测HHT频谱中能观测到一定程度的地震前兆异常,各分量的优势频率大部分在0.01 Hz,但并不是距震中300 km内的每个台站的地磁相对观测分量HHT频谱中都能明...     

地磁HHT频谱分析在地震预测中的应用

利用希尔伯特-黄变换方法,对成都、重庆、拉萨地磁台记录到的汶川M_S 8.0地震、汶川地震余震地磁数据进行分析处理,发现在4级及以上中强度地震前3个月内地磁相对观测HHT频谱中能观测到一定程度的地震前兆异常,各分量的优势频率大部分在0.01 Hz,但并不是距震中300 km内的每个台站的地磁相对观测分量HHT频谱中都能明显地观测到异常,这可能与台站所处的构造位置有关。     

高压直流输电对泾县地震台地磁观测干扰分析

高压直流输电线路对地磁观测的干扰幅度大,随意性大.泾县地震台地磁观测目前受到附近穿行的多条高压直流输电影响,且无法避免.通过对泾县地震台观测资料分析,就高压直流输电对地磁观测的干扰原理和一些识别的方法有一定认识,并掌握有效剔除方法.     

辽宁省地震局召开“三连冠”表奖大会

辽宁省地震局于1986年10月20日在大连市召开了对大连地震台和金州地震台的表奖大会。大连地震台的地磁观测工作,在基础较差的条件下,克服重重困难、奋起直追。在1983年,1984年和1985年的全国地磁观测资料质量评比中,连续三届获得地磁三类台第一名,并荣获司南奖杯。金州地震台的短水准观测工作,自建台以来,克服各种困难,坚持高标准、严要求。     

九寨沟MS7.0地震前地磁异常

分析距离九寨沟M_S7.0地震震中分别为65 km、254 km和238 km的松潘地磁台、成都地磁台和天水地磁台2017年连续观测结果,发现九寨沟地震前,松潘地磁台出现异常变化,主要表现为2017年5月开始,松潘地磁台长时间垂直分量累积变化量达40 nT。短时间内也存在地磁场突变,最高可达10 nT,而成都地磁台和天水地磁台地磁场无明显异常。通过对观测数据的详细检查发现松潘地磁台很多观测日的最后一个观测值与后一观测日的第一个观测值相差超过1 nT,因此认为九寨沟地震前观测数据的异常是由观测系统异常导致。对三个台站地磁场垂直分量日变化的统计分析发现垂直分量在不同时段相关性保持一致,说明地震前短时间内不存在地磁垂直分量的明显异常变化,三个台站地磁场日变化的差异是由地下介质性质不同导致。岩石圈磁场在震中西侧区域出现正负异常交替现象,这可能与九寨沟地震的孕育有关。     

泾县地震台地磁核旋观测干扰排除分析

地磁观测是地震预报中重要的前兆手段之一。识别干扰,排除干扰,对保证观测资料的可靠尤为重要。我们根据泾县地震台地磁核旋观测过程中遇到的问题,利用对比观测方法,对观测数据进行分析,结果表明该仪器工作正常,性能稳定,精度很高;同时指出,在观测过程中应注意的一些问题,并排除了影响泾县地震台地磁观测的干扰源。     

On the synchronism in the events within the core and on the surface of the earth: the changes in the organic world and in the polarity of the geomagnetic field in the phanerozoic

The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes in the organic world.     

On the maintenance of the axisymmetric part of the flow in the atmosphere

Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan.     

On the gravimetric undulations of the geoid and the deflections of the vertical

Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out.     

太平洋中部地磁台11年周期变化的研究

综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后,可定性地提出该变化源于内场。如内源为核幔边界的电涡流,则其中心点应位于3台之间。     

Magnetic stratigraphy of the Ordovician in the lower reach of the Kotuy River: the age of the Bysy-Yuryakh stratum and the rate of geomagnetic reversals on the eve of the superchron

Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.     

On the variation in the geomagnetic dipole over the geological history of the Earth

The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data.     

Comparison Between the Nutations of the Planet Mars and the Nutations of the Earth

The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth.     

Evolutionary Changes in the Configuration of the Magnetic Field of the Solar Corona in the Epoch of the Minimum

Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the...